EDP Sciences
Free Access
Issue
A&A
Volume 559, November 2013
Article Number A12
Number of page(s) 14
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/201221012
Published online 29 October 2013

Online material

thumbnail Fig. 3

Abundance ratios [X/Fe] for aluminum and α-elements versus [Fe/H]. The data were taken from Luck & Heiter (2007) (black crosses); Reddy et al. (2006) (green crosses); Fulbright (2000) (red crosses); Gratton & Sneden (1991), and For & Sneden (2011) (blue crosses). CD-41°15048 and HD 214362 are represented by black squares.

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thumbnail Fig. 4

Abundance ratios [X/Fe] for the iron group elements versus [Fe/H]. Symbols have the same meaning as in Fig. 3.

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thumbnail Fig. 5

Abundance ratios [X/Fe] for the heavy elements. Symbols have the same meaning as in Fig. 3, except for zirconium and lanthanum. For zirconium we used the results of Edvardsson et al. (1993) (black crosses), and for lanthanum we used the results of Mishenina et al. (2006) (black crosses).

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thumbnail Fig. 8

Same as in Fig. 7, but in the YZ plane.

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thumbnail Fig. 10

Same as in Fig. 9, but in the YZ plane.

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thumbnail Fig. 11

Same as in Fig. 7, but for BD+09°3223 in the XY plane. The present position is labeled with “X”.

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thumbnail Fig. 12

Same as in Fig. 11, but in the YZ plane.

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Table 1

Observed Fe i and Fe ii lines.

Table 3

Other lines studied.

Table 5

Abundance uncertainties for CD-41°15048.


© ESO, 2013

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